Predictions of the L-[C ii]-SFR and [Cii] Luminosity Function at the Epoch of Reionization
Research output: Contribution to journal › Journal article › peer-review
We present the first predictions for the L-[C ii]-SFR relation and [Cii] luminosity function (LF) in the epoch of reionization (EOR) based on cosmological hydrodynamics simulations using the simba suite plus radiative transfer calculations via sigame. The sample consists of 11,137 galaxies covering halo mass log M-halo [9, 12.4] M, star formation rate SFR [0.01, 330] M yr(-1), and metallicity Z(gas)(SFR) [0.1, 1.9] Z. The simulated L-[C ii]-SFR relation is consistent with the range observed, but with a spread of 0.3 dex at the high end of SFR (>100 M yr(-1)) and 0.6 dex at the lower end, and there is tension between our predictions and the values of L-[C ii] above 10(8.5) L observed in some galaxies reported in the literature. The scatter in the L-[C ii]-SFR relation is mostly driven by galaxy properties, such that at a given SFR galaxies with higher molecular mass and metallicity have higher L-[C ii]. The [Cii] LF predicted by simba is consistent with the upper limits placed by the only existing untargeted flux-limited [Cii] survey at the EOR and those predicted by semianalytic models. We compare our results with existing models and discuss the differences responsible for the discrepant slopes in the L-[C ii]-SFR relation.
Original language | English |
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Article number | 102 |
Journal | Astrophysical Journal |
Volume | 905 |
Issue number | 2 |
Number of pages | 16 |
ISSN | 0004-637X |
DOIs | |
Publication status | Published - 1 Dec 2020 |
- Galaxy evolution, Galactic and extragalactic astronomy, Galaxy properties, Interstellar emissions, Interstellar medium, Hydrodynamical simulations, Radiative transfer simulations, STAR-FORMING GALAXIES, C-II, MOLECULAR GAS, LINE EMISSION, DUST CONTENT, BLACK-HOLE, X-RAYS, SIMULATIONS, ALMA, REDSHIFT
Research areas
Links
- https://arxiv.org/pdf/2004.11912.pdf
Submitted manuscript
ID: 254460871